A Sasakian metric is defined using the construction of the Riemannian cone. Given a Riemannian manifold, its Riemannian cone is the product of with a half-line, equipped with the cone metric where is the parameter in. A manifold equipped with a 1-form is contact if and only if the 2-form on its cone is symplectic. A contact Riemannian manifold is Sasakian, if its Riemannian cone with the cone metric is a Kähler manifold with Kähler form
Examples
As an example consider where the right hand side is a natural Kähler manifold and read as the cone over the sphere. The contact 1-form on is the form associated to the tangent vector, constructed from the unit-normal vector to the sphere. Another non-compact example is with coordinates endowed with contact-form and the Riemannian metric As a third example consider: where the right hand side has a natural Kähler structure, and the group acts by reflection at the origin.
History
Sasakian manifolds were introduced in 1960 by the Japanese geometer Shigeo Sasaki. There was not much activity in this field after the mid-1970s, until the advent of String theory. Since then Sasakian manifolds have gained prominence in physics and algebraic geometry, mostly due to a string of papers by Charles P. Boyer and Krzysztof Galicki and their co-authors.
The homothetic vector field on the cone over a Sasakian manifold is defined to be As the cone is by definition Kähler, there exists a complex structureJ. The Reebvector field on the Sasaskian manifold is defined to be It is nowhere vanishing. It commutes with all holomorphic Killing vectors on the cone and in particular with all isometries of the Sasakian manifold. If the orbits of the vector field close then the space of orbits is a Kähler orbifold. The Reeb vector field at the Sasakian manifold at unit radius is a unit vector field and tangential to the embedding.
Sasaki–Einstein manifolds
A Sasakian manifold is a manifold whose Riemannian cone is Kähler. If, in addition, this cone is Ricci-flat, is called Sasaki–Einstein; if it is hyperkähler, is called 3-Sasakian. Any 3-Sasakian manifold is both an Einstein manifold and a spin manifold. If M is positive-scalar-curvature Kahler–Einstein manifold, then, by an observation of Shoshichi Kobayashi, the circle bundle S in its canonical line bundle admits a Sasaki–Einstein metric, in a manner that makes the projection from S to M into a Riemannian submersion. While this Riemannian submersion construction provides a correct local picture of any Sasaki–Einstein manifold, the global structure of such manifolds can be more complicated. For example, one can more generally construct Sasaki–Einstein manifolds by starting from a Kahler–Einstein orbifoldM. Using this observation, Boyer, Galicki, and János Kollár constructed infinitely many homeotypes of Sasaki-Einstein 5-manifolds. The same construction shows that the moduli space of Einstein metrics on the 5-sphere has at least several hundred connected components.